Figure 2 from The Solar Probe ANalyzers—Electrons on the Parker Solar Probe

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The Solar Probe ANalyzers—Electrons on the Parker Solar Probe

Authors: Phyllis L. Whittlesey, Davin E. Larson, Justin C. Kasper, Jasper Halekas, Mamuda Abatcha, Robert Abiad, M. Berthomier, A.W. Case, Jianxin Chen, David W. Curtis, Gregory Dalton, Kristopher G. Klein, Kelly E. Korreck, Roberto Livi, Michael Ludlam, Mario Marckwordt, Ali Rahmati, Miles Robinson, Amanda Slagle, M.L. Stevens, Chris Tiu, and J.L. Verniero

2020 The Astrophysical Journal Supplement Series 246 74.

Provider: AAS Journals

Caption: Figure 2.

The two SPAN-E Sensors’ individual FOVs, overlaid on the same sky map. The blue trace is the extent of the SPAN-Ae FOV, and the orange is for the SPAN-B sensor. The red trace describes intrusions to SPAN-B’s FOV by the spacecraft, and the dark blue trace, intrusions to SPAN-Ae. Identifiable features include the magnetic field instrument boom, two FIELDs antennas, and the high gain antenna. The Sun is at (0, 0), and the ram-direction is at (90, 0).

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